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XRISM is set to observe NGC 1365 twice during the initial PerformanceVerification Phase for a total of 250 ks. Here we request two simultaneousXMM-Newton (2 i??i?? 120 ks) and NuSTAR (2x60 ks) observations that will greatlyenhance the science output of these observations. While XRISM willprobe the ionized wind with unprecedented en- ergy resolution with the additionof XMM-Newton we can probe the variability of that outflow onshort timescales. Moreover XMM-Newton will enable simultaneous measurements ofthe broad iron line and potential reverberation lags allowing us to understand how the inner accretion flow and highly ionized outflowsinteract. One of XMM- Newtoni??i??i??s legacies has been to reveal time variability [truncated! Please see actual data for full text]